Signals of Neutralino Dark Matter from Earth and Sun
arXiv:hep-ph/9408391 · doi:10.1016/0927-6505(94)00028-2
Abstract
We evaluate the fluxes of up--going muons detectable in a neutrino telescope and due to the annihilation of relic neutralinos in the Earth and in the Sun, taking realistically into account the fact that neutralinos might provide only a fraction of the local (solar neighbourhood) dark matter (DM). We determine the relation between the exposure of the neutrino telescope ( being the telescope area, the live time) and the explorable range of the neutralino mass and composition, when the signal--to--background ratio is optimized by an appropriate angular selection.
14 pages in Plain TeX, 14 figures included in a separate uuencoded tarred-compressed Postscript file; Report number: DFTT 34/95; To appear in Astroparticle Physics
References in corpus (4)
Cited by in corpus (41)
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